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Home > Mathematics and Science Textbooks > Science: general issues > A Manual of Spherical and Practical Astronomy, Embracing the General Problems of Spherical Astronomy Volume 1; The Special Applications to Nautical Astronomy, and the Theory and Use of Fixed and Portable Astronomical Instruments
A Manual of Spherical and Practical Astronomy, Embracing the General Problems of Spherical Astronomy Volume 1; The Special Applications to Nautical Astronomy, and the Theory and Use of Fixed and Portable Astronomical Instruments

A Manual of Spherical and Practical Astronomy, Embracing the General Problems of Spherical Astronomy Volume 1; The Special Applications to Nautical Astronomy, and the Theory and Use of Fixed and Portable Astronomical Instruments


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This historic book may have numerous typos and missing text. Purchasers can download a free scanned copy of the original book (without typos) from the publisher. Not indexed. Not illustrated. 1868 Excerpt: ...follow the right ascension of the moon's limb at the instants of transit over the two meridians, taking in each case the mean value found from all the stars observed. Put Lv La = the approximate or assumed longitudes, 1 = the true difference of longitude, o os = the observed right ascensions of the moon's bright limb at 2/, and La respectively, H0 = the variation of the E. A. of the moon's limb for 1 of longitude while passing from Ll to La; then we have in which, otg--a, and H0 being both expressed in seconds, X will be in hours and decimal parts. When the difference of longitude is less than two hours, it is found to be sufficiently accurate to regard H0 as constant, provided we employ its value for the middle longitude L0 = i(Lt + L2), found by interpolation from the values in the Ephemeris, having regard to second differences. Example.--The following observations were made, May 15. 1851, at Santiago, Chili, by the U. S. Astronomical Expedition under Lieut. Gilliss, and at Philadelphia, by Prof. Kendall: We shall assume the longitudes from Greenwich to be, Philadelphia, i, = 5 0-39'.85 Santiago, L = 4 42 19. the longitude of Philadelphia being that which results from the last chronometric expeditions of the U. S. Coast Survey, and that of Santiago the value which Lieut. Gilliss at first assumed. The apparent right ascensions of the stars on May 15, by the moon-culminating list in the Nautical Almanac, were and a' and b0 are found from the values of H in the Ephemeris as follows: Mayl5, L.C. 142-.56 2ddiff "15, TIC. 143.48 + _0..28 + 0.64-0.35 which is the longitude of Santiago from Philadelphia. Ileneo, if the longitude of Philadelphia is correct, we have Long, of Santiago = 4 42TM 33'.95 from Greenwich. 233. Corresponding observations ...


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Product Details
  • ISBN-13: 9781236114426
  • Publisher: Rarebooksclub.com
  • Publisher Imprint: Rarebooksclub.com
  • Height: 246 mm
  • No of Pages: 164
  • Spine Width: 9 mm
  • Width: 189 mm
  • ISBN-10: 1236114426
  • Publisher Date: 01 May 2012
  • Binding: Paperback
  • Language: English
  • Returnable: N
  • Weight: 304 gr


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A Manual of Spherical and Practical Astronomy, Embracing the General Problems of Spherical Astronomy Volume 1; The Special Applications to Nautical Astronomy, and the Theory and Use of Fixed and Portable Astronomical Instruments
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